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6081. http://hea-www.harvard.edu/ChandraSNR/SNRJ0106.2-7205/9100/work/snr104_sou.pi.par
xswabs[xswabs] (XSPEC model name : wabs) ( integrate : off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.2768 1e-07 10 10^22/cm^2 xsvmekal[xsvmekal] (XSPEC model name : vmekal) ( integrate : on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 kT thawed 0.6546 1e-03 100 keV 2 nH frozen 1 1e-06 1e+20 per cm**3 3 He frozen 1 0 1000 with respect to ...
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0106.2-7205/9100/work/snr104_sou.pi.par -- 2.8 Кб -- 14.01.2010
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6082. http://hea-www.harvard.edu/ChandraSNR/G001.9+00.3/6708/work/g019_sou.pi.par
xswabs[xswabs] (XSPEC model name : wabs) ( integrate : off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 3.9144 1e-07 10 10^22/cm^2 xsvmekal[xsvmekal] (XSPEC model name : vmekal) ( integrate : on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 kT thawed 95.4129 1e-03 100 keV 2 nH frozen 1 1e-06 1e+20 per cm**3 3 He frozen 1 0 1000 with respect to ...
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Ссылки http://hea-www.harvard.edu/ChandraSNR/G001.9+00.3/6708/work/g019_sou.pi.par -- 2.8 Кб -- 14.01.2010
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6083. http://hea-www.harvard.edu/ChandraSNR/SNRJ0550.4-6823/3850/work/snr0550_sou.pi.par
xswabs[xswabs] (XSPEC model name : wabs) ( integrate : off) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 nH thawed 0.3164 1e-07 10 10^22/cm^2 xsvmekal[xsvmekal] (XSPEC model name : vmekal) ( integrate : on) Param Type Value Min Max Units ----- ---- ----- --- --- ----- 1 kT thawed 0.2334 1e-03 100 keV 2 nH frozen 1 1e-06 1e+20 per cm**3 3 He frozen 1 0 1000 with respect to ...
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNRJ0550.4-6823/3850/work/snr0550_sou.pi.par -- 2.8 Кб -- 14.01.2010
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6084. http://hea-www.harvard.edu/~alexey/emulateapj/emulateapj-rtx4.cls
... For release notes and change log, see at bottom %% %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% \ def \emulapj@ver{08/22/09} \ProvidesClass{emulateapj} \newif\if@two@col \DeclareOption{twocolumn}{\@two@coltrue} \DeclareOption{onecolumn ... \bibbaselineskip}\setlength{\bibbaselineskip}{3.075mm} \newif\if@apj@letter \DeclareOption{apj}{ \setlength{\bibbaselineskip}{2.7mm} \ def \apjsecfont{\normalsize} \ def \secnum@size{\small} \ ... B$}}% % U-B \newcommand\bv{\mbox{$B\!- ...
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Ссылки http://hea-www.harvard.edu/~alexey/emulateapj/emulateapj-rtx4.cls -- 57.9 Кб -- 10.11.2009
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6085. http://hea-www.harvard.edu/AstroStat/Stat310_0910/ds_20091103.pdf
Classification of Sunspot Groups Using SOHO/MDI Magnetogram and White-Light Images Tuesday, November 3, 2009 Background/Motivation Ї Sunspot classification is (for the most part) done manually by experts in the field. ... Tuesday, November 3, 2009 The Plan An automatic sunspot detection and classification procedure will be developed using SOHO/MDI magnetogram and whitelight images. ... Tuesday, November 3, 2009 Then, we cut out a region on the white-light image that matches the magnetogram. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_0910/ds_20091103.pdf -- 449.9 Кб -- 03.11.2009
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_0910/ds_20091103.pdf -- 449.9 Кб -- 03.11.2009
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_0910/ds_20091103.pdf -- 449.9 Кб -- 03.11.2009
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6086. http://hea-www.harvard.edu/AstroStat/Stat310_0910/ab_20091103.pdf
Outline Problem Previous approaches Proposed method Results on MACHO data Extensions Robust Wavelet Models for Event Detection in Time Series Databases Alexander W Blocker Pavlos Protopapas 3 November, 2009 Outline Problem Previous approaches Proposed method Results on MACHO data Extensions Outline Problem Previous approaches Proposed Our goal is to identify and characterize time series containing events. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_0910/ab_20091103.pdf -- 650.9 Кб -- 03.11.2009
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_0910/ab_20091103.pdf -- 650.9 Кб -- 03.11.2009
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_0910/ab_20091103.pdf -- 650.9 Кб -- 03.11.2009
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6087. http://hea-www.harvard.edu/AstroStat/Stat310_0910/jx_20091103.pdf
... T. Solar DEM Model Proposal E(Ib ) i 1 i t 1 I T t M b it i : the volume (abundance?) of ion i t : the proportion of the total volume at temperature t Solar Dataset Ї 15 Filters.txt files: The temperature response of each of the Hinode/XRT filter combinations With column 1 being the temperature in log10([K]) and column 2 being the expected rate [DN/s] for an isothermal Emission Measure of 1e25 cm^-5/pix. ... The dataset doesn't seem quite fit the previous Solar DEM model. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_0910/jx_20091103.pdf -- 452.4 Кб -- 03.11.2009
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_0910/jx_20091103.pdf -- 452.4 Кб -- 03.11.2009
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_0910/jx_20091103.pdf -- 452.4 Кб -- 03.11.2009
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6088. http://hea-www.harvard.edu/vlp_m33_public/ic131_102909.pdf
... Although the corresponding X-ray spectrum has 1215 counts, it cannot conclusively be told whether the extended X-ray emission is thermal, non-thermal, or a combination of both. A thermal plasma model of k Te = 4.3 keV or a single power law of 2.1 fit the spectrum equally well. If the spectrum is purely thermal (non-thermal), the total unabsorbed X-ray luminosity in the 0.35 ґ 8 keV energy band amounts to LX = 6.8 (8.7) в 1035 erg s-1 . ... Is the X-ray emission non-thermal? ...
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Ссылки http://hea-www.harvard.edu/vlp_m33_public/ic131_102909.pdf -- 1615.2 Кб -- 29.10.2009
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6089. http://hea-www.harvard.edu/AstroStat/Stat310_0910/bck_20091006.pdf
... 2009 10/6/09 AstrostaCsCcsClass HierarchicalModelforDustMaps Ї UseBayesianhierarchical modeltosimultaneously log Ci ~ N ( ?C ,VC ) modelthejoint T ~ p(T | ... f ) n i= 1 J N (log Ci | ... Missing Data Included Data 10/6/09 AstrostaCsCcsClass PosteriorDistribuCon Ї TheobserveddatalikelihoodisfoundbyintegraCngoverthe missingdata: p( I, x obs | ... Included Data p( I = 1 | ... dx Ї Assumingapriorp(N,)=p()/N(i.e.,uniformonlogN),the marginalposteriorofis(e.g.,Gelmanetal.,2004) p( | ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_0910/bck_20091006.pdf -- 2277.8 Кб -- 21.10.2009
[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_0910/bck_20091006.pdf -- 2277.8 Кб -- 21.10.2009
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[ Текст ] Ссылки http://hea-www.harvard.edu/astrostat/Stat310_0910/bck_20091006.pdf -- 2277.8 Кб -- 21.10.2009
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6090. http://hea-www.harvard.edu/~bradw/cv/papers/whiteGenX.pdf
... Complex astrophysical phenomena could now be studied spectroscopically: the X-ray absorption line forest intrinsic to Seyfert galaxies; the interaction between AGN jets and intracluster media; hot winds of starburst galaxies; stellar coronal plasmas; the charge -exchange emission of Mars' exosphere; the X-ray irradiation of protoplanetary disks; and the myst erious flat-topped spectral line shapes of O star winds. ... We estimate that Gen-X will be able to detect and resolve 20, 000 stars in NGC...
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Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/whiteGenX.pdf -- 434.2 Кб -- 08.10.2009
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6091. http://hea-www.harvard.edu/~bradw/cv/papers/whiteIXO.pdf
... Introduction It may seem counterintuitive that X-ray astronomy should give any insights into planetary systems: planets, and their natal protoplanetary disks (PPDs), have temperatures which are far to o co ol (100 - 1500 K) to emit X-rays. ... The resulting X-ray emission gives unique insights into the solar activity, planetary atmospheres, cometary comae, charge exchange physics, and space weather across the Solar System (review by Bhardwa j et al. 2007). ... 2007; Gudel 2007). ... 2007, Planet. ...
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Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/whiteIXO.pdf -- 1012.8 Кб -- 08.10.2009
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6092. http://hea-www.harvard.edu/ChandraSNR/G010.0-00.3/746/work/region_description
psr.reg=Pulsar pwn.reg=Halo
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Ссылки http://hea-www.harvard.edu/ChandraSNR/G010.0-00.3/746/work/region_description -- 1.0 Кб -- 24.08.2009
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6093. http://hea-www.harvard.edu/ChandraSNR/G033.6+00.1/1982/work/region_description
snr.reg=total a1.reg= a2.reg= a3.reg= a4.reg= a5.reg= a6.reg=
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Ссылки http://hea-www.harvard.edu/ChandraSNR/G033.6+00.1/1982/work/region_description -- 1.1 Кб -- 24.08.2009
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6094. http://hea-www.harvard.edu/ChandraSNR/G042.8+00.6/1954/work/region_description
psr.reg=The SGR point source halo.reg=Dust-scattered halo
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Ссылки http://hea-www.harvard.edu/ChandraSNR/G042.8+00.6/1954/work/region_description -- 1.1 Кб -- 24.08.2009
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6095. http://hea-www.harvard.edu/ChandraSNR/G054.1+00.3/1983/work/region_description
snr.reg=total psr.reg=central source pwn.reg=pulsar-wind nebula diff.reg=faint diffuse emission
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Ссылки http://hea-www.harvard.edu/ChandraSNR/G054.1+00.3/1983/work/region_description -- 1.1 Кб -- 24.08.2009
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6096. http://hea-www.harvard.edu/ChandraSNR/SNR0506-68.0/2762/work/region_description
snr.reg=total sh.reg=shell a1.reg=bright interior patch, SW a2.reg=bright interior patch, S a3.reg=bright interior patch, SE
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Ссылки http://hea-www.harvard.edu/ChandraSNR/SNR0506-68.0/2762/work/region_description -- 1.1 Кб -- 24.08.2009
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6097. http://hea-www.harvard.edu/~bradw/cv/papers/penning.pdf
installed at the AXAF X-ray Calibration Facility at Marshall 2. ... On theoretical grounds, we expect this line to be even nar3 0.04 rower than measured, but in any case, it will serve very well for calibrating the MEG resolution. ... Spectrum of the Penning source with 0.02A bins. ... D. S. Finley, S. Bowyer, F. Paresce, and R. F. Malina, "Continuous discharge Penning source with emission lines between 50 A and 300 A", Appl. ...
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Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/penning.pdf -- 15.9 Кб -- 05.08.2009
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6098. http://hea-www.harvard.edu/~bradw/cv/papers/bubble2.pdf
Separating Local and Cosmic Soft X-ray Emission in the Chandra Deep Field-South B.J. Wargelin, M. Juda, and J.D. Slavin Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 Abstract. The Chandra Deep Field-South (CDF-S) observing program, comprising 2 Ms of data collected near Solar Maximum (1999 and 2000) and during Solar Minimum (2007), provides a uniquely rich and informative data set for investigation of solar wind charge exchange (SWCX) and the soft X-ray background (SXRB). ...
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Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/bubble2.pdf -- 120.1 Кб -- 23.07.2009
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6099. http://hea-www.harvard.edu/PINTofALE/pro/rd_list.pro
... Returning',/informational return,-1L endif ;ss='[ ' + STRING(9B) + ']+' ; default separator (one or more sp or tab ) ss=' ' ; default separator if keyword_ set ( sep ) then ss= sep pfx='*' ; default comment prefix if keyword_ set (prefix) then pfx=string(prefix) mm=0 ; default mapping of multiple matches nm=n_elements(mapping) szm=size(mapping) nszm=n_elements(szm) if nm gt 0 then begin mm=1 ;MAPPING has been ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/pro/rd_list.pro -- 16.9 Кб -- 14.05.2009
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6100. http://hea-www.harvard.edu/PINTofALE/pro/mk_dem.pro
... TYPE can be ; 'help' ; 'constant' PARDEM = value ; 'chebyshev' PARDEM = coefficients ; 'cursor' PARDEM = max range in DEM ; 'interpolate' PARDEM = original logT ; 'loop' PARDEM = original logT ; 'rebin' PARDEM = rebinning scales ; 'spline' PARDEM = logT location of points ; 'varsmooth' PARDEM = smoothing scales ; 'delta' PARDEM = logT locations of EM components ; if a particular method requires an input ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/pro/mk_dem.pro -- 14.4 Кб -- 13.04.2009
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